Probability of occurrence of planetary ionosphere storms associated with the magnetosphere disturbance storm time events

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Abstract

The ionospheric W index allows to distinguish state of the ionosphere and plasmasphere from quiet conditions (W Combining double low line 0 or ±1) to intense storm (W Combining double low line ±4) ranging the plasma density enhancements (positive phase) or plasma density depletions (negative phase) regarding the quiet ionosphere. The global W index maps are produced for a period 1999-2014 from Global Ionospheric Maps of Total Electron Content, GIM-TEC, designed by Jet Propulson Laboratory, converted from geographic frame (-87.5:2.5:87.5° in latitude, -180:5:180° in longitude) to geomagnetic frame (-85:5:85° in magnetic latitude, -180:5:180° in magnetic longitude). The probability of occurrence of planetary ionosphere storm during the magnetic disturbance storm time, Dst, event is evaluated with the superposed epoch analysis for 77 intense storms (Dst ≤-100 nT) and 230 moderate storms (-100 < Dst -50 nT) with start time, t0, defined at Dst storm main phase onset. It is found that the intensity of negative storm, iW-, exceeds the intensity of positive storm, iW+, by 1.5-2 times. An empirical formula of iW+ and iW- in terms of peak Dst is deduced exhibiting an opposite trends of relation of intensity of ionosphere-plasmasphere storm with regard to intensity of Dst storm.

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Gulyaeva, T. L., Arikan, F., & Stanislawska, I. (2014). Probability of occurrence of planetary ionosphere storms associated with the magnetosphere disturbance storm time events. Advances in Radio Science, 12, 261–266. https://doi.org/10.5194/ars-12-261-2014

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